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Paleomagnetic evidence for Neoarchean plate mobilism

Ding, Jikai ; Rogers, Chris ; Söderlund, Ulf LU ; Evans, David A.D. ; Gong, Zheng ; Ernst, Richard E. ; Chamberlain, Kevin and Kilian, Taylor (2024) In Nature Communications 15(1).
Abstract

Plate tectonics is a unique feature of Earth, but its proposed time of initiation is still controversial, with published estimates ranging from ca. 4.2 to 0.7 Ga. Paleomagnetic data can provide a robust argument for one essential aspect of plate tectonics: large-scale relative lateral motions of distinct, rigid crustal blocks. Previously, the oldest relative horizontal motion between two or more blocks was constrained to a broad age interval of ca. 2.7–2.17 Ga using paleomagnetic data. In this study, we obtain a robust ca. 2.48 Ga paleomagnetic pole from Wyoming craton. Combining this result with the ca. 2.7–2.17 Ga apparent polar wander paths from Wyoming and Superior cratons, we suggest that they assembled during ca. 2.7–2.5 Ga and... (More)

Plate tectonics is a unique feature of Earth, but its proposed time of initiation is still controversial, with published estimates ranging from ca. 4.2 to 0.7 Ga. Paleomagnetic data can provide a robust argument for one essential aspect of plate tectonics: large-scale relative lateral motions of distinct, rigid crustal blocks. Previously, the oldest relative horizontal motion between two or more blocks was constrained to a broad age interval of ca. 2.7–2.17 Ga using paleomagnetic data. In this study, we obtain a robust ca. 2.48 Ga paleomagnetic pole from Wyoming craton. Combining this result with the ca. 2.7–2.17 Ga apparent polar wander paths from Wyoming and Superior cratons, we suggest that they assembled during ca. 2.7–2.5 Ga and remained directly juxtaposed until ca. 2.17 Ga. Tectonostratigraphic data and geological proxies also suggest Wyoming and Superior collided at ca. 2.6 Ga. The results provide strong evidence for relative horizontal motion between crustal blocks during the Neoarchean. Together with other tectonic proxies, the data suggest plate mobilism in operation prior to 2.5 Ga.

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Contribution to journal
publication status
published
subject
in
Nature Communications
volume
15
issue
1
article number
10814
publisher
Nature Publishing Group
external identifiers
  • scopus:85213725404
  • pmid:39737974
ISSN
2041-1723
DOI
10.1038/s41467-024-55117-w
language
English
LU publication?
yes
id
182a7196-0fa8-4e3a-875c-8753b60818cc
date added to LUP
2025-02-26 10:43:06
date last changed
2025-06-04 18:50:35
@article{182a7196-0fa8-4e3a-875c-8753b60818cc,
  abstract     = {{<p>Plate tectonics is a unique feature of Earth, but its proposed time of initiation is still controversial, with published estimates ranging from ca. 4.2 to 0.7 Ga. Paleomagnetic data can provide a robust argument for one essential aspect of plate tectonics: large-scale relative lateral motions of distinct, rigid crustal blocks. Previously, the oldest relative horizontal motion between two or more blocks was constrained to a broad age interval of ca. 2.7–2.17 Ga using paleomagnetic data. In this study, we obtain a robust ca. 2.48 Ga paleomagnetic pole from Wyoming craton. Combining this result with the ca. 2.7–2.17 Ga apparent polar wander paths from Wyoming and Superior cratons, we suggest that they assembled during ca. 2.7–2.5 Ga and remained directly juxtaposed until ca. 2.17 Ga. Tectonostratigraphic data and geological proxies also suggest Wyoming and Superior collided at ca. 2.6 Ga. The results provide strong evidence for relative horizontal motion between crustal blocks during the Neoarchean. Together with other tectonic proxies, the data suggest plate mobilism in operation prior to 2.5 Ga.</p>}},
  author       = {{Ding, Jikai and Rogers, Chris and Söderlund, Ulf and Evans, David A.D. and Gong, Zheng and Ernst, Richard E. and Chamberlain, Kevin and Kilian, Taylor}},
  issn         = {{2041-1723}},
  language     = {{eng}},
  number       = {{1}},
  publisher    = {{Nature Publishing Group}},
  series       = {{Nature Communications}},
  title        = {{Paleomagnetic evidence for Neoarchean plate mobilism}},
  url          = {{http://dx.doi.org/10.1038/s41467-024-55117-w}},
  doi          = {{10.1038/s41467-024-55117-w}},
  volume       = {{15}},
  year         = {{2024}},
}